Asymmetric drift in MaNGA: mass and radially dependent stratification rates in galaxy discs

Bershady, Matthew A.; Westfall, Kyle B.; Shetty, Shravan; Law, David R.; Cappellari, Michele; Drory, Niv; Bundy, Kevin; Yan, Renbin

doi:10.1093/mnras/stae1207

Title: Asymmetric drift in MaNGA: mass and radially dependent stratification rates in galaxy discs

Journal Article · 06 May 2024 · Monthly Notices of the Royal Astronomical Society

DOI: https://doi.org/10.1093/mnras/stae1207 · OSTI ID:2361187

; Westfall, Kyle B.; Shetty, Shravan; Law, David R.;

; Drory, Niv; Bundy, Kevin; Yan, Renbin

ABSTRACT We measure the age–velocity relationship from the lag between ionized gas and stellar tangential speeds in ∼500 nearby disc galaxies from MaNGA in Sloan Digital Sky Survey IV (SDSS-IV). Selected galaxies are kinematically axisymmetric. Velocity lags are asymmetric drift, seen in the Milky Way’s (MW) solar neighbourhood and other Local Group galaxies; their amplitude correlates with stellar population age. The trend is qualitatively consistent in rate ($$\dot{\sigma }$$) with a simple power-law model where σ ∝ tb that explains the dynamical phase-space stratification in the solar neighbourhood. The model is generalized based on disc dynamical times to other radii and other galaxies. We find in-plane radial stratification parameters σ0,r (dispersion of the youngest populations) in the range of 10–40 km s−1 and 0.2 < br < 0.5 for MaNGA galaxies. Overall, brincreases with galaxy mass, decreases with radius for galaxies above 10.4 dex (M⊙) in stellar mass, but is ∼constant with radius at lower mass. The measurement scatter indicates the stratification model is too simple to capture the complexity seen in the data, unsurprising given the many possible astrophysical processes that may lead to stellar population dynamical stratification. None the less, the data show dynamical stratification is broadly present in the galaxy population, with systematic trends in mass and density. The amplitude of the asymmetric drift signal is larger for the MaNGA sample than the MW, and better represented in the mean by what is observed in the discs of M31 and M33. Either typical discs have higher surface-density or, more likely, are dynamically hotter (hence thicker) than the MW.

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Sponsoring Organization:: USDOE

OSTI ID:: 2361187

Journal Information:: Monthly Notices of the Royal Astronomical Society, Journal Name: Monthly Notices of the Royal Astronomical Society Journal Issue: 1 Vol. 531; ISSN 0035-8711

Publisher:: Oxford University PressCopyright Statement

Country of Publication:: United Kingdom

Language:: English

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The SDSS-IV MaNGA Sample: Design, Optimization, and Usage Considerations Wake, David A.; Bundy, Kevin; Diamond-Stanic, Aleksandar M. The Astronomical Journal, Vol. 154, Issue 3 https://doi.org/10.3847/1538-3881/aa7ecc	journal	August 2017
The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Emission-line Modeling Belfiore, Francesco; Westfall, Kyle B.; Schaefer, Adam The Astronomical Journal, Vol. 158, Issue 4 https://doi.org/10.3847/1538-3881/ab3e4e	journal	September 2019
The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview Westfall, Kyle B.; Cappellari, Michele; Bershady, Matthew A. The Astronomical Journal, Vol. 158, Issue 6 https://doi.org/10.3847/1538-3881/ab44a2	journal	November 2019
SDSS-IV MaNGA: Modeling the Spectral Line-spread Function to Subpercent Accuracy Law, David R.; Westfall, Kyle B.; Bershady, Matthew A. The Astronomical Journal, Vol. 161, Issue 2 https://doi.org/10.3847/1538-3881/abcaa2	journal	January 2021
The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age Quirk, Amanda C. N.; Guhathakurta, Puragra; Gilbert, Karoline M. The Astronomical Journal, Vol. 163, Issue 4 https://doi.org/10.3847/1538-3881/ac5324	journal	March 2022
Asymmetric Drift in the Andromeda Galaxy (M31) as a Function of Stellar Age Quirk, Amanda; Guhathakurta, Puragra; Chemin, Laurent The Astrophysical Journal, Vol. 871, Issue 1 https://doi.org/10.3847/1538-4357/aaf1ba	journal	January 2019
Stellar Population Synthesis with Distinct Kinematics: Multiage Asymmetric Drift in SDSS-IV MaNGA Galaxies Shetty, Shravan; Bershady, Matthew A.; Westfall, Kyle B. The Astrophysical Journal, Vol. 901, Issue 2 https://doi.org/10.3847/1538-4357/ab9b8e	journal	September 2020
SDSS-IV MaNGA: Refining Strong Line Diagnostic Classifications Using Spatially Resolved Gas Dynamics Law, David R.; Ji, Xihan; Belfiore, Francesco The Astrophysical Journal, Vol. 915, Issue 1 https://doi.org/10.3847/1538-4357/abfe0a	journal	July 2021
Dynamical Model of the Milky Way Using APOGEE and Gaia Data Nitschai, Maria Selina; Eilers, Anna-Christina; Neumayer, Nadine The Astrophysical Journal, Vol. 916, Issue 2 https://doi.org/10.3847/1538-4357/ac04b5	journal	August 2021
The TREX Survey: Kinematical Complexity Throughout M33's Stellar Disk and Evidence for a Stellar Halo* Gilbert, Karoline M.; Quirk, Amanda C. N.; Guhathakurta, Puragra The Astrophysical Journal, Vol. 924, Issue 2 https://doi.org/10.3847/1538-4357/ac3480	journal	January 2022
The ALMaQUEST Survey. VIII. What Causes the Discrepancy in the Velocity between the CO and Hα Rotation Curves in Galaxies? Su, Yung-Chau; Lin, Lihwai; Pan, Hsi-An The Astrophysical Journal, Vol. 934, Issue 2 https://doi.org/10.3847/1538-4357/ac77fd	journal	August 2022
The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution Experiment Abolfathi, Bela; Aguado, D. S.; Aguilar, Gabriela The Astrophysical Journal Supplement Series, Vol. 235, Issue 2 https://doi.org/10.3847/1538-4365/aa9e8a	journal	April 2018
The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data The Astrophysical Journal Supplement Series, Vol. 259, Issue 2, p. 35 https://doi.org/10.3847/1538-4365/ac4414	journal	March 2022
Pipe3D, a pipeline to analyze Integral Field Spectroscopy data: I. New fitting phylosophy of FIT3D Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P. arXiv https://doi.org/10.48550/arXiv.1509.08552	preprint	January 2015
Pipe3D, a pipeline to analyse integral field spectroscopy data: II. Analysis sequence and CALIFA dataproducts Sánchez, S. F.; Pérez, E.; Sánchez-Blázquez, P. arXiv https://doi.org/10.48550/arXiv.1602.01830	preprint	January 2016
SSDSS IV MaNGA - Properties of AGN host galaxies Sanchez, S. F.; Avila-Reese, V.; Hernandez-Toledo, H. arXiv https://doi.org/10.48550/arXiv.1709.05438	preprint	January 2017

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